Solar Activity Waiting Time Distribution Function for Different Spatial and Temporal Scales Phenomena

  • Adolfo L. Méndez Berhondo Instituto de Geofísica y Astronomía, Calle 212 No. 2906 entre 29 y 31, La Coronela, La Lisa, Ciudad de La Habana, CP 11 600
  • Ramón E. Rodríguez Taboada Instituto de Geofísica y Astronomía, Calle 212 No. 2906 entre 29 y 31, La Coronela, La Lisa, Ciudad de La Habana, CP 11 600

Abstract

In this work we search for waiting time distribution function of two kind of solar transient events characterized both by its different spatial and temporal scales: solar radio spikes and coronal mass ejections with two emissions. We found that in both the distribution seems to follow a power-law. This paper summarizes the works presented in the workshop Complexity 2006 in Havana Cuba, referred to solar physics.

Published
Dec 1, 2006
How to Cite
MÉNDEZ BERHONDO, Adolfo L.; RODRÍGUEZ TABOADA, Ramón E.. Solar Activity Waiting Time Distribution Function for Different Spatial and Temporal Scales Phenomena. Revista Cubana de Física, [S.l.], v. 23, n. 2, p. 93-96, dec. 2006. ISSN 2224-7939. Available at: <https://revistacubanadefisica.org/index.php/rcf/article/view/RCF_23_2_93>. Date accessed: 20 apr. 2024.
Citation Formats
Issue
Vol 23 No 2 (2006)
Section
Original Articles

This work is licensed under the Creative Commons Attribution-NonCommercial 4.0 International (CC BY-NC 4.0) license.